Ship's Log: Collaborative East Antarctic Marine Census
On board the Aurora Australis, Voyage Leader, Dr Martin Riddle, captured the excitement of the CEAMARC sea-bed surveys in his 'situation reports'. The voyage also supported another Australian-led International Polar Year project – Climate of Antarctica and the Southern Ocean (CASO).
DATE: 21/12/07 POSITION: -62 48E, 142 51S ICE CONDITIONS: nil
In transit to the main sampling area for both CEAMARC and the southern CASO sites. The third Continuous Plankton Recorder tow is currently in the water. Yesterday afternoon the first bulk seawater sample was collected for metagenomic analysis using techniques based on those developed for sequencing the human genome.
DATE: 23/12/07 POSITION: -65 59E, 142 39.6S ICE CONDITIONS: 2/10 loose pack ice
An octopus (left) glides through an underwater garden of corals, sponges and starfish.
Photo: AAD
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DATE: 25/12/07 POSITION: -66 20E, 143 17S ICE CONDITIONS: distant icebergs
A trawl-mounted camera provided tantalising video footage of the sea-bed.
Photo: AAD
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DATE: 28/12/07 POSITION: -66 33S, 143 19E ICE CONDITIONS: continent in sight
Giant glass sponges from the Antarctic can grow to 1.5 m tall.
Photo: AAD
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DATE: 03/01/08 POSITION: -66 34S, 144 41E ICE CONDITIONS: distant icebergs
After riding out 40 to 50 knot winds for the first day and a half of the New Year, conditions had abated sufficiently by 1600 hrs yesterday to allow sampling to re-commence. Overall impressions of the sea-bed invertebrate communities are that the diversity and species composition on the Adélie Bank seems roughly equivalent to that known from at Dumont D'Urville at shallower depths (40-200 m), but tends to decrease in Commonwealth Bay, possibly because of increased iceberg scouring. Two stations (38 and 36) show strikingly different benthic communities compared to surrounding stations, with many anemones, synascidians and serolid isopods. These stations are situated well beneath the action of icebergs at the bottom of the Georges V Basin where water conditions may play a role in shaping very different assemblages. The multi-beam data, previously collected in this area by the US research vessel the Nathaniel Palmer, provides a very detailed picture of the sea-bed, including tracks of past iceberg scouring . The data is proving invaluable for interpreting the relationship between the living communities and the physical environment of the sea-bed.
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DATE: 04/01/08 POSITION: -66 19S, 143 59E ICE CONDITIONS: isolated bergs
At 23 cm long, 9 cm wide and 330 gm in weight, this scale worm was larger than any previously seen by the biologists on board.
Photo: AAD
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DATE: 06/01/08 POSITION: -65 39.6S, 143 02.4E ICE CONDITIONS: isolated bergs, bergy bits
We all expected the Big Polychaete to be the undisputed highlight of the voyage, however, the Southern Ocean continues to turn-up surprises. Yesterday, while sampling the transect from 400 m to 2100 m down the shelf, we blew out the trawl net as we tried to bring it on deck after sampling the 800 m site. The video footage from the trawl-mounted camera explained why. Almost the entire day shift crammed into the electronics cupboard to see the footage and, after the first gasps of 'incroyable!', watched in hushed awe as a scene rivalling the best parts of the Great Barrier Reef was revealed. The sea-bed was 100% covered with living material – colourful branching coralline species and gorgonians forming the major lower storey structure and large branching sponges the upper storey. Amongst this were numerous sea-stars, sea-cucumbers, crustacea and fish of types at yet unseen. After repairing the trawl nets we returned to re-sample the site, this time being very cautious with the time allowed for the trawl to be on the bottom, and were rewarded with a relatively small catch, but with many species not previously collected. In marked contrast the communities at 1600 m and 2100 m were rather sparse, with much un-colonised rock and coarse sediment visible, but again the samples, although small, contained many species new to us. The deck crew must be congratulated for their skill and persistence in successfully sampling these very difficult environments, without which the scientists would have nothing. We have now commenced the main CASO (Climate of Antarctica and the Southern Ocean) sampling for the voyage.
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At 800m on the edge of the continental slope (left) a reef of cold water corals, gorgonians and sponges provided a habitat for a rich community, including fish, crustaceans and sea stars. Biodiversity between 1600 and 2000 m (right) was sparse in comparison to shallower depths, with much bare rock. But even at these depths species new to the survey were found, such as the dark red deep sea prawn (right of image).
DATE: 08/01/08 POSITION: -62 58S, 145 44E ICE CONDITIONS: open water
Conductivity, Temperature and Depth (CTD) sampling bottles.
Photo: Sandra Potter
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DATE: 13/01/08 POSITION: -66 03.7, 141 17.7E ICE CONDITIONS: large icebergs, open water
A diverse collection of sponges from the CEAMARC voyage.
Photo: AAD
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DATE: 15/01/08 POSITION: -66 24.4, 139 47.6E ICE CONDITIONS: icebergs, bergy bits, growlers
Diatomaceous ooze at 1200 m proved difficult to sample, but supported a range of species.
Photo: AAD
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DATE: 19/01/08 POSITION: -65 37, 141 04.3E ICE CONDITIONS: large iceberg, bergy bits, growlers
As predicted, sampling the very rugged seabed in this canyon system at the edge of the continental shelf has been difficult. At the cost of some torn trawl nets, we have managed to get imagery and samples down to 1500 m, with the very diverse seabed offering up a similarly diverse fauna. Last night we recorded the most fish species from any one trawl - 16 including at least one which was new to this survey. The benthic invertebrates were similarly diverse with a great range of sedentary groups, such as sponges, bryozoans (lace coral), tunicates (sea squirts), gorgonians and some very large solitary corals, forming the main supporting structure for an equally diverse variety of mobile groups such as polychaete worms, amphipod crustaceans, ophuroids (brittle stars), crinoids (feather stars), echinoids (sea urchins), asteroids (sea stars), pycnogonids (sea spiders) and a range of molluscs. Early this morning we stopped the benthic work temporarily and switched our efforts to sampling the waters around the very large iceberg nearby, with the intention of identifying whether it is a source of trace nutrients that might stimulate plankton growth. Satellite imagery indicates the iceberg is about 35 km long by 18 km wide. The berg is designated B-17A and came into this region in October 2006 from a large chunk of the Ross Ice Shelf that calved in April 2000.
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DATE: 20/01/08 POSITION: -65 24.7, 139 50.7E ICE CONDITIONS: open water
Yesterday water samples were collected from seven sites at a range of distances from the large iceberg using the Fast Rescue Craft. While sampling was happening, the Aurora Australis maintained its position down-wind and down-current to ensure there was no risk of the ship contaminating the surface waters. These samples are to be analysed for ultra-low levels of trace elements and even the presence of the ship's hull in the immediate sampling area could compromise the results . The CEAMARC sampling officially finished at 12:08 am. Overall, 82 different sites were occupied during CEAMARC, with samples collected from at least 78 sites; well in excess of the 67 sites we had hoped for. Everyone involved is to be congratulated for putting in an enormous and sustained effort to achieve such an excellent result.
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Sampling for CEAMARC began at site 27 and continued around the George V Basin, concluding at site 67 some two weeks later. Sampling for CASO then began (dotted arrows). CEAMARC sampling around the Adélie Bank and Basin continued about one week later from site 1. (Map No. 13475) |
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More information:
To read the full sitreps visit the Aurora Australis voyage on the Census of Antarctic Marine Life website.
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